Results are presented from two balloon flights of an ionization/Cerenkov detector system. Well-defined peaks at nickel (Z = 28) and zinc (Z = 30) yield abundances relative to iron (Z = 26) of 0.05 and 0.006, respectively. About sixty events observed in the interval yield abundances relative to iron similar to those of the standard solar-system.
Cosmic-ray abundances in the interval 26 is less than or equal to Z is less than or equal to 40
International Cosmic Ray Conference ; 1979 ; Kyoto, Japan
1980-01-01
Miscellaneous
No indication
English
European Patent Office | 2015
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